Dam Nuisance

 fieldwork  Comments Off
Sep 262008
 
We are here

We are here

Last year I helped compile a geotrail for the Churnet Valley in Staffordshire, England. Just as we were about to publish the trail I discovered that a key footbridge had been closed temporarily. This involved a hasty rewrite including an alternate route. I went back this week to see if it had reopened. It hasn’t, but it is now clearer why it is shut – the dam beneath the footbridge is failing.

To set the scene, the area is situated in the Upper Carboniferous, Bashkirian (Westphalian) Coal Measures which were extensively mined for both coal and ironstone. The Froghall Ironstone used to outcrop on the western side of the valley shown in the map below. The spoil, predominantly red siltstones, from ironstone mines on the western side of the valley were used to build an embankment across the valley to take a tramway from coal and ironstone mines further up on the eastern side of the valley. The valley was dammed and a lake formed up stream. It is this spoil dam that is now disintegrating.


View Larger Map

In recent times, the embankment was replaced with a footbridge and a spillway from the lake forming a stream under the bridge as can be seen in this photograph taken last year. Just above the stream bed is intact siltstone bedrock but soon passes upwards into loose spoil.

Dam spillway, Mosey Moor Wood, August 2007

Dam spillway, Mosey Moor Wood, August 2007

A view from the other side of the bridge last summer shows siltstone spoil underneath the eastern bridge support.

Dam spillway, Mosey Moor Wood, September 2007

Dam spillway, Mosey Moor Wood, September 2007

Now contrast this with the scene yesterday.

Dam Spillway, Mosey Moor Wood, September 2008

Dam Spillway, Mosey Moor Wood, September 2008

There is now no water flowing through the spillway as the lake level above the dam is below the spillway lip. Instead, the water is now flowing through the dam spoil material itself and the spoli is being washed out in the process, and further undermining the bridge support.

Fortunately, there is another, intact, tramway embankment a few hundred metres downstream of this dam which should buffer the effects should the dam totally fail and the lake drain catastrophically.

 

Time Scale - after Chris Rowan

Time Scale - after Chris Rowan

Chris at Good Schist is hosting this month’s Accretionary Wedge #13: Geology in Space.

I think that I should preface this piece by saying that I’m not a planetary scientist and this just my understanding, and I apologise for any inaccuracies in advance. If you stumble across this piece via a search engine and want too use this for research / an essay may your god help you.

Something catastrophic may (or may not*) have happened during the Cambrian on Venus.

The timescale (adapted from Chris Rowan at Highly Allochtonous) on the left shows the sort of time I’m dealing with here, about 500 Ma ago.

The surface ages of a planetary body are dated by crater counting, the older the surface, the more the craters (and the larger the craters) are. By this measure, Venus appears to have an usually uniform crater density and most craters are fresh and little degraded implying that Venus underwent a planet-wide resurfacing episode at about 500 Ma. The easiest way to resurface a planet is to flood it with volcanic lava, 80% of the plains of Venus are lava flows and there are over 50,000 volcanoes in nearly 650 volcanic fields mapped on the surface of Venus. The large volcanic structures appear to post-date the resurfacing – yet no volcanoes are seen erupting today and most would be considered extinct.

USGS)

Volcanos on Venus (source: USGS)

The implication is that during the Cambrian there was a massive volcanic episode with the outpourings of lava almost completely obliterating what went before, and then the volcanism stopped just as abruptly.

As a further clue to what might have happened we need to look more closely at a couple of other surface features on Venus, the highlands and chasmae.

NASA]

Surface features of Venus as radar mapped by Magellan (Source: NASA)

The highlands in this Magellan radar image, colour coded according to elevation are yellow, for example Ovda Regio and Thetis Regio in the centre right of the image. Below Thetis Regio is the circular chasm of Artemis Chasma.

Nasa)

Tessera terrain, Eistla Regio, Venus (Source: Nasa)

The highlands of Venus stand about 2 – 4 km higher than the surrounding volcanic plains and from the crater count they are slightly older. They are dissected by often orthogonal ridges and grooves produced by a complex history of compression and extension, giving rise to what is known as tessera terrain (a tessera being a tile in a mosaic).

In extensional faulting, the separation of the faults is characteristic of the depth of brittle / ductile transition. The scale of the tesserae (about 5-20 km across) can be used to imply a relatively shallow aesthenoshere / lithosphere detachment ~10km, perhaps unsurprising for a hot planet with a surface temperature in the highlands of 374°C (lowlands 465°C).

NASA)

Coranae and chasma (Source: NASA)

The chasmae on the younger lowlands are associated with the margins corona structures, believed to be large diapiric upwellings. The extension related chasmae, a couple of kilometres deep, have profiles which from modelling of the four main coronae gives lithospheric elastic thicknesses of 15, 40, 37 & 35 km which are comparable to Earth (25 km Hawaii – 50 km subduction zones). These large elastic thicknesses require low thermal gradients (<10°C/km – half the expected) and a thicker lithosphere to when the highlands were created.

Unknown)

Venus Lithosphere Change (Source: Unknown)

So, lithosphere thickness may have changed dramatically with time due to a change in convection by planetary cooling. In this theory highlands are emplaced just before the switch, with a thin lithosphere and prolific magmatism. Volcanic rises are emplaced after the change with thick lithosphere and low magmatism. The change-over appears to be rapid as there are no transitional forms. [Apologies for not linking the source of the above image - if anyone knows it leave a comment].

If this process occurred then is it a process that is common in terrestrial style planet thermal evolution? Could rapid lithospheric thickening happen on Earth changing the tectonic style? Or has it already happened?

[*Note: some more recent authors (e.g. here and here) now dispute the timing of this catastrophe or that there was a massive volcanic outpouring at all. Although they don't seem to preclude a catastrophic event at 500 Ma, models also allow a more steady state resurfacing.]

 
Satnalls Hills Quarry

Satnalls Hills Quarry

The good news is that I’ve been given a grant to compile a geological trail for Cannock Chase, Staffordshire, UK. However, I’ve just checked back and I started the grant application process back at the end of April and only I found out the result last Friday (and I still haven’t got the official confirmation yet). The trail has to be completed and printed by the end of February. I restart teaching the week after next so I’ve only got one week to get the fieldwork done (well finished anyway, as I have been doing some work in the mean time hoping that the grant would come off). Fortunately, not only has the grant arrived, but so has the British summer at long last – just in time for Autumn.

Pebbles, pebbles and more pebbles

Pebbles, pebbles and more pebbles

Cannock Chase is predominantly Triassic pebbles from a large braided river system unconformably overlying Carboniferous Coal Measures. The area has been quarried for gravel and mined for coal. There is also an interesting glacial history. However, most of the area is covered either by heathland or forest. Exposures are few and far between so a geological trail is going to be challenging.

Coal Measures to left, Triassic to right

Eastern Boundary Fault: Coal Measures to left, Triassic to right

Mineral Meme Redux

 memes  Comments Off
Sep 102008
 

Callan and Nova Geoblog has subverted the Minerals Meme with the question …

Which five minerals do you think are the most important ones to know, and why? In other words, if you had to introduce a non-geologist to just five of the earth’s multitudinous building blocks, which ones would you choose to share, and offer a justification for each.

You can see Callan’s favourite five here and Kim at All My Faults list is here. Like Kim, I’ve tried not to look at the previous posts until I’ve finished my five.

1. Perovskite

From the 660km spinel to perovskite transition at the upper/lower mantle boundary down to the core/mantle boundary at 2900km the Earth’s lower mantle is dominated by perovskite (or at least the pyroxene enstatite with a perovskite structure). By my calculations, the lower mantle comprises about 55% of the Earth by volume, making this the Earth’s commonest mineral.

My Ph.D. was on deep earthquakes so I developed a keen interest in mantle structure and mineralogy.

2. Olivine

For similar reasons, olivine has to be one of the fundamental minerals, dominating the upper mantle. I also think that it is also one of the most vibrant when seen under the microscope in cross-polarised light. I’d better add a passing reference to spinel here. As much as I’m interested in mantle minerals, I don’t want to waste all my five.

3. Iron

Whilst the outer core is liquid and not technically a mineral, the inner core is solid. There is some evidence from the seismic anisotropy of the inner core that it (or maybe the inner-inner core) is crystalline iron, possibly even a single crystal!

4. Quartz

Quartz is probably the most logical choice. Being stable, it is a common component of igneous, sedimentary and metamorphic rocks are found pretty much everywhere. If there is one mineral that is common at the Earth’s surface, this is it. Passing mention should go to feldspars, not quite as common due to their being less stable but again found in many igneous (even more than quartz), sedimentary and metamorphic rocks.

5. Calcite

Calcite is important not only as the main constituent of limestone but because it locks up so much CO2 from the atmosphere. If we didn’t have calcite, our atmosphere would be full of CO2 from volcanoes and we would be a greenhouse planet like Venus.

OK, lets see how I compare
Callan has 1. Quartz, 2. Clays, 3. Olivine (+spinel +perovskite), 4. Plagioclase, 5 Ice.
Kim has 1. Quartz, 2. Calcite, 3. Pyrite, 4. Clays, 5. Olivine

I suppose it is unsurprising that we come up with similar lists. I suspect that my geophysics / seismology background makes me think a little ‘deeper’, but we are all on pretty much the same wavelength.

Not too sure about ice though. Sure it is technically a mineral but it smacks a bit too much of geography.

 

Chuck at the Lounge of the Lab Lemming has started a Fifty Great Minerals Meme.

Minerals in bold for those seen in the wild, italic for lab/museum/non-field.

Without further ado, here are mine…

50 minerals everyone should see:

Andalucite
Apatite
Barite
Beryl
Biotite
Chromite
Chrysotile
Cordierite
Corundum
Diamond
Dolomite
Florencite
Galena
Garnet
Graphite
Gypsum
Halite
Hematite
Hornblende
Illite
Illmenite
Kaolinite
Kyanite
Lepidolite
Limonite
Magnetite
Molybdenite
Monazite
Nepheline
Olivine
Omphacite
Opal
Perovskite
Plagioclase
Pyrite
Quartz
Rutile
Sanidine
Sillimanite
Silver (native)
[but Gold (native)]
Sphalerite
Staurolite
Sulphur (native)
Talc
Tourmaline
Tremolite
Turquoise
Vermiculite
Willemite
Zeolite
Zircon

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